Gravitational waves from oscillons in a generalized exponential plateau potential
Peter Lott, Tuan Q. Do
astro-ph.CO, gr-qc
Submitted: 2026-07-31
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Pseudo-Stable Bubbles
- Oscillons: Resonant Configurations During Bubble Collapse
- Reheating after Inflation
- Towards the Theory of Reheating After Inflation
- Structure of Resonance in Preheating after Inflation
- Analytical Characterization of Oscillon Energy and Lifetime
- Flat-top oscillons in an expanding universe
- Oscillons After Inflation
- Radiation and Relaxation of Oscillons
- Inflaton Fragmentation and Oscillon Formation in Three Dimensions
- Self-resonance after inflation: oscillons, transients and radiation domination
- Enhancement of Gravitational Waves Induced by Scalar Perturbations due to a Sudden Transition from an Early Matter Era to the Radiation Era
- Numerical Gaussian process Kalman filtering
- Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies
- Detecting High-Frequency Gravitational Waves with Microwave Cavities
- The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters
- The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models
- Inflation from a generalized exponential plateau: towards extra suppressed tensor-to-scalar ratios
- Planck 2018 results. VI. Cosmological parameters
- Gravitational Wave Experiments and Early Universe Cosmology
Related papers
- Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
- A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
- Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
- Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
- Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation